The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS
arXiv:0803.1504 · doi:10.1086/588042
Abstract
We present c2d Spitzer/IRAC observations of the Lupus I, III and IV dark clouds and discuss them in combination with optical and near-infrared and c2d MIPS data. With the Spitzer data, the new sample contains 159 stars, 4 times larger than the previous one. It is dominated by low- and very-low mass stars and it is complete down to M 0.1M. We find 30-40 % binaries with separations between 100 to 2000 AU with no apparent effect in the disk properties of the members. A large majority of the objects are Class II or Class III objects, with only 20 (12%) of Class I or Flat spectrum sources. The disk sample is complete down to ``debris''-like systems in stars as small as M 0.2 M and includes sub-stellar objects with larger IR excesses. The disk fraction in Lupus is 70 -- 80%, consistent with an age of 1 -- 2 Myr. However, the young population contains 20% optically thick accretion disks and 40% relatively less flared disks. A growing variety of inner disk structures is found for larger inner disk clearings for equal disk masses. Lupus III is the most centrally populated and rich, followed by Lupus I with a filamentary structure and by Lupus IV, where a very high density core with little star-formation activity has been found. We estimate star formation rates in Lupus of 2 -- 10 M Myr and star formation efficiencies of a few percent, apparently correlated with the associated cloud masses.
arXiv commentAccepted for publication in the ApJS. Contains 101 pages, 23 figures, and 13 tables. A version with full resolution figures can be found at http://peggysue.as.utexas.edu/SIRTF/PAPERS/pap102.pub.pdf
References in corpus (37)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- Embedded Clusters in Molecular Clouds
- The Spitzer Space Telescope Mission
- Dust Grain Size Distributions and Extinction in the Milky Way, LMC, and SMC
- Disk Frequencies and Lifetimes in Young Clusters
- Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
- Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
- The Formation of a Star Cluster: Predicting the Properties of Stars and Brown Dwarfs
- From Molecular Cores to Planet-forming Disks: A SIRTF Legacy Program
- Accretion Disks Around Young Objects. II. Tests of Well-Mixed Models with Ism Dust
- Observations of IC348: The Disk Population at 2-3 Million Years
- The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K
- 2-D Radiative Transfer in Protostellar Envelopes: II. An Evolutionary Sequence
- IRAC Observations of Taurus Pre-Main Sequence Stars
- Dust dynamics during protoplanetary disc clearing
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. III. Perseus Observed with IRAC
- The Spitzer c2d Survey of Weak-line T Tauri Stars II: New Constraints on the Timescale for Planet Building
- The Initial Configuration of Young Stellar Clusters: A K-band Number Counts Analysis of the Surface Density of Stars
- The Spitzer c2d Survey of Large, Nearby, Insterstellar Clouds. IX. The Serpens YSO Population As Observed With IRAC and MIPS
- Cold Disks: Spitzer Spectroscopy of Disks around Young Stars with Large Gaps
- Binarity as a key factor in protoplanetary disk evolution: Spitzer disk census of the eta Chamaeleontis cluster
- Young, Low-Mass Brown Dwarfs with Mid-Infrared Excesses
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds.X. The Chamaeleon II Pre-Main Sequence Population as Observed With IRAC and MIPS
- Empirical isochrones and relative ages for young stars, and the radiative-convective gap
- Medium-separation binaries do not affect the first steps of planet formation
- SPITZER: Accretion in Low Mass Stars and Brown Dwarfs in the Lambda Orionis Cluster
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. I. Chamaeleon II Observed with MIPS
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds VIII. Serpens Observed with MIPS
- New Low-Mass Stars and Brown Dwarfs with Disks in Lupus
- Giant Planet Migration in Viscous Power-Law Discs
- The Spitzer c2d survey of Large, Nearby, Interstellar Clouds. V. Chamaeleon II Observed with IRAC
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. IV. Lupus Observed with MIPS
- Mass loss at the lowest stellar masses
- Abundant crystalline silicates in the disk of a very low mass star
- Very low-mass members of the Lupus 3 cloud
- WWW Database of Models of Accretion Disks Irradiated by The Central Star
- Automatic quenching of high energy gamma-ray sources by synchrotron photons
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- The Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes
- The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
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- ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses
- The Disk Substructures at High Angular Resolution Project (DSHARP): II. Characteristics of Annular Substructures
- X-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects
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- X-Shooter spectroscopy of young stellar objects: IV -- Accretion in low-mass stars and sub-stellar objects in Lupus
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- X-Shooter spectroscopy of young stellar objects: II. Impact of chromospheric emission on accretion rate estimates
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- A Spitzer c2d Legacy Survey to Identify and Characterize Disks with Inner Dust Holes
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- The evolution of dust-disk sizes from a homogeneous analysis of 1-10 Myr-old stars
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- The Luminosities of Protostars in the Spitzer c2d and Gould Belt Legacy Clouds
- The Spitzer Survey of Interstellar Clouds in the Gould Belt. III. A Multi-Wavelength View of Corona Australis
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- A Herschel Survey of Cold Dust in Disks Around Brown Dwarfs and Low-Mass Stars
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- The Nature of Transition Circumstellar Disks II. Southern Molecular Clouds
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- The Spitzer survey of interstellar clouds in the Gould Belt. II. The Cepheus Flare observed with IRAC and MIPS
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- Substellar Objects in Nearby Young Clusters (SONYC) IX: The planetary-mass domain of Chamaeleon-I and updated mass function in Lupus-3
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- Probing the Final Stages of Protoplanetary Disk Evolution with ALMA
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- POISSON project - III - Investigating the evolution of the mass accretion rate
- Transition disks: the observational revolution from SEDs to imaging
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- A Census of the Circumstellar Disk Populations in the Sco-Cen Complex
- New Herbig Ae/Be stars confirmed via high-resolution optical spectroscopy
- Substellar Objects in Nearby Young Clusters (SONYC) VIII: Substellar population in Lupus 3
- Identification of new transitional disk candidates in Lupus with Herschel
- ALMA Survey of Lupus Class III Stars: Early Planetesimal Belt Formation and Rapid Disk Dispersal
- Evolution of the T Tauri star population in the Lupus association
- The effect of stellar multiplicity on protoplanetary discs. A NIR survey of the Lupus star forming region
- The diagnostic potential of Fe lines applied to protostellar jets
- Photometric determination of the mass accretion rates of pre-main sequence stars. III. Results in the Large Magellanic Cloud
- Herschel evidence for disk flattening or gas depletion in transitional disks
- Gas inside the 97 au cavity around the transition disk Sz\,91
- A Gaia Survey for Young Stars Associated with the Lupus Clouds
- Populations of Young Stellar Objects in Nearby Molecular Clouds
- What happened before? -- The disks around the precursors of young Herbig Ae/Be stars
- Constraining the radial drift of millimeter-sized grains in the protoplanetary disks in Lupus
- The Spitzer Survey of Interstellar Clouds in the Gould Belt. VI. The Auriga-California Molecular Cloud observed with IRAC and MIPS
- Multi-wavelength study of the disk around the very low-mass star Par-Lup3-4
- The Spitzer Survey of Interstellar Clouds in the Gould Belt. V. Ophiuchus North Observed with IRAC and MIPS
- The VISTA Orion mini-survey: star formation in the Lynds 1630 North cloud
- ESO-H~574 and Par-Lup3-4 Jets: Exploring the spectral, kinematical and physical properties
- Gaia DR2 view of the Lupus V-VI clouds: the candidate diskless young stellar objects are mainly background contaminants
- Multi-line spectral imaging of dense cores in the Lupus molecular cloud
- ALMA observations of the Th 28 protostellar disk - A new example of counter-rotation between disk and optical jet
- The Spitzer Survey of Interstellar Clouds in the Gould Belt. IV. Lupus V and VI Observed with IRAC and MIPS
- The Supershell-Molecular Cloud Connection: Large-Scale Stellar Feedback and the Formation of the Molecular ISM
- A proper motion study of the Lupus clouds using VO tools
- The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
- X-Shooter spectroscopy of young stellar objects - VI - HI line decrements
- The viscous evolution of circumstellar discs in young star clusters
- Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25
- Large-Scale CO Maps of the Lupus Molecular Cloud Complex
- Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs
- Squeezed between shells? On the origin of the Lupus I molecular cloud. APEX/LABOCA, Herschel, and Planck observations
- The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): III. Dust and Gas Disk Properties in the Lupus Star-forming Region
- Outflows in rho Ophiuchi as Seen with the Spitzer Infrared Array Camera
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- Search for Alignment of Disk Orientations in Nearby Star-Forming Regions: Lupus, Taurus, Upper Scorpius, Ophiuchi, and Orion
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- ALMA observations of the early stages of substellar formation in the Lupus 1 and 3 molecular clouds
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- The Power of SOFIA/FORCAST in Estimating Internal Luminosities of Low Mass Class 0/I Protostars
- New X-ray Selected Pre-Main Sequence Members of the Serpens Molecular Cloud